1. Residual Background events after Rejection Cuts 119.6 M total background events (GlastReleasev3r3p7) 344 residual events after Bill's rejection cuts. 342 events were studied using the gui, MeritTuple and Mc Root Data. (The other 2 events are missing because the corresponding root files are corrupt). Luis Reyes - 03.22.04

2. Surprise... (~36 events like this one) Preliminary analysis indicates that displayed primary particle is not consistent with McXDir, McYDir, McZDir from ntuple.

3. From Mc Root File: (this is the complete Mc tree, no “pruning” was done, Heather made a special run of this event) Lines are drawn using the initial and final position from Mc File Dashed line is based on initial momentum from Mc File. Consistent with McXDir,... Red=Proton Yellow=gamma Blue=electron Black box is an approx. of the volume of the LAT.

4. The bug is not always senseless... ` Conclusions: The algorithm to write the final position is messing up (~85 events) when the primary particle is interacting but not losing its identity. It's not a good idea to draw the primary particle using the final position only, the particle can be scattering in between. This is actually the final Position Wrong Trajectory Red=Proton Gray=neutron Blue=electron (Right trajectory shown by green arrows)

5. Calculating the Background Rate A background average rate of 4.2 Khz/m^2 was assumed. 4.2 KHz / m^2 * 6 m^2 = 25.2 KHz picked up by Glast 119.6M events correspond to an elapsed time of 4746.03 s 344 events / 4746.03 s = 0.0725 Hz

6. Interactions in the Blanket e +   p Protons scatter inelastically from the blanket. We get backgrounds when the particles thrown in the tracker direction are neutral and there no ACD hits. 50 events (15%) Positrons with energies around 150 MeV annihilate producing two gammas. 39 events (11%) 0.0105 Hz 0.0082 Hz

7. Hadron Showers p->X in spacecraft or Cal No clear MIP signature.  + 70 events (20%) Same as above but either the primary particle or one of the daughters leaves a MIP signature in the CAL. 64 events (19%) 0.0147 Hz 0.0135 Hz Extra activity in Tkr may be useful. CAL pattern?

8. e interactions + e + Take place at the spacecraft or CAL 33 events (10%) Albedo Gammas 35 events (10%) 0.0074 Hz 0.0070 Hz

9. Tkr1SSDVeto Criteria Events where the ACD was fired up are allowed with the condition that Tkr1SSDVeto>2 (so that backsplash gammas are kept). However, the track might be pointing to the wrong tile. Tkr1SSDVeto≡ # of live SSD back along trajectory from start of first track to ACD 22 events (6%) 0.0046 Hz Tkr1SSDVeto = 6 E=513.2 MeV

10. ACD Cracks e + 10 events are protons (3%) 0.0021 Hz 19 events are e, (6%) 0.0040 Hz e + In some occasions a tile is marginally hit in the gui but no ActDist is calculated. Reducing the threshold may get some of these events rejected.

11. Summary Table Blanket (p) 15 % 0.0105 Hz 0.0082 Hz 0.0147 Hz 0.0135 Hz 0.0070Hz 0.0046 Hz 0.0021 Hz 0.0040 Hz 0.0074 Hz 11 % 20 % 19 % 10 % 6 % 3 % 6 % 10 % Blanket (e) Hadron Shower Hadron Shower with MIP e Interactions TkrSSDVeto Criteria Acd Crack (p) Acd Crack (e) Albedo Gamma Type Percentage out of 342 Bgnd Rate